Probing the very high energy γ-ray spectral curvature in the blazar PG 1553+113 with the MAGIC telescopes
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ-ray emitter classified as a BL Lac object. Its redshift is constrained by intergalactic absorption lines in the range 0.4
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Veröffentlicht in: | Monthly Notices of the Royal Astronomical Society 2015-07, Vol.450 (4), p.4399-4410 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ-ray emitter classified as a BL Lac object. Its redshift is constrained by intergalactic absorption lines in the range 0.4 |
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ISSN: | 0035-8711 1365-2966 |
DOI: | 10.1093/mnras/stv811 |